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  2. OJ 287 - Wikipedia

    en.wikipedia.org/wiki/OJ_287

    OJ 287 is a BL Lac object 4 billion light-years from Earth that has produced quasi-periodic optical outbursts going back approximately 120 years, as first apparent on photographic plates from 1891.

  3. Messier 81 - Wikipedia

    en.wikipedia.org/wiki/Messier_81

    Messier 81 (also known as NGC 3031 or Bode's Galaxy) is a grand design spiral galaxy about 12 million light-years away in the constellation Ursa Major. It has a D 25 isophotal diameter of 29.44 kiloparsecs (96,000 light-years ).

  4. NGC 4889 - Wikipedia

    en.wikipedia.org/wiki/NGC_4889

    At the core of the galaxy is a supermassive black hole that heats the intracluster medium through the action of friction from infalling gases and dust. The gamma ray bursts from the galaxy extend out to several million light years of the cluster. As with other similar elliptical galaxies, only a fraction of the mass of NGC 4889 is in the form ...

  5. Dark galaxy - Wikipedia

    en.wikipedia.org/wiki/Dark_galaxy

    A dark galaxy is a hypothesized galaxy with no (or very few) stars. They received their name because they have no visible stars but may be detectable if they contain ...

  6. Black Eye Galaxy - Wikipedia

    en.wikipedia.org/wiki/Black_Eye_Galaxy

    The Black Eye Galaxy (also called Sleeping Beauty Galaxy or Evil Eye Galaxy and designated Messier 64, M64, or NGC 4826) is a relatively isolated [7] spiral galaxy 17 million light-years away in the mildly northern constellation of Coma Berenices.

  7. Sombrero Galaxy - Wikipedia

    en.wikipedia.org/wiki/Sombrero_Galaxy

    The Sombrero Galaxy (also known as Messier Object 104, M104 [4] or NGC 4594) is a peculiar galaxy of unclear classification [5] in the constellation borders of Virgo and Corvus, being about 9.55 megaparsecs (31.1 million light-years) [2] from the Milky Way galaxy.

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  9. NGC 7727 - Wikipedia

    en.wikipedia.org/wiki/NGC_7727

    In November 2021, scientists announced the discovery of a pair of supermassive black holes in NGC 7727, detected with the Very Large Telescope's multi-unit spectroscopic explorer (MUSE) at the European Southern Observatory. The black holes have masses of 154 and 6.3 million solar masses, and are separated 1,600 light years apart.

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